1SWASP J030749.87-365201.7 , the SIMBAD biblio

1SWASP J030749.87-365201.7 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.05.29CEST20:49:02

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Bibcode/DOI Score in Title|Abstract|
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2011A&A...528A..90N viz 15       D               1 61 58 Short period eclipsing binary candidates identified using SuperWASP. NORTON A.J., PAYNE S.G., EVANS T., et al.
2012A&A...542A.124L 16       D               2 55 31 Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit. LOHR M.E., NORTON A.J., KOLB U.C., et al.
2013A&A...549A..86L viz 16       D               1 155 48 Period and period change measurements for 143 SuperWASP eclipsing binary candidates near the short-period limit and discovery of a doubly eclipsing quadruple system. LOHR M.E., NORTON A.J., KOLB U.C., et al.
2016AJ....151..168K 16       D               3 50 1 Multi-filter light curves of 29 very short period candidate contact binaries. KOEN C., KOEN T. and GRAY R.O.
2017MNRAS.469.3688D viz 16       D               1 37714 19 The Catalina Surveys Southern periodic variable star catalogue. DRAKE A.J., DJORGOVSKI S.G., CATELAN M., et al.
2019MNRAS.485.4588L 17       D               1 57 ~ Contact binaries at the short period cut-off - I. Statistics and the first photometric investigations of 10 totally eclipsing systems. LI K., XIA Q.-Q., MICHEL R., et al.
2020MNRAS.497.3493Z 17       D               1 358 ~ Orbital period cut-off of W UMa-type contact binaries. ZHANG X.-D. and QIAN S.-B.
2021ApJS..254...10L viz 18       D               1 692 ~ Statistics of 700 individually studied W UMa stars. LATKOVIC O., CEKI A. and LAZAREVIC S.
2022RAA....22b5011Z 47           X         1 10 ~ CSS J075415.6+191052 and NW Leo: Two Contact Binaries at Different Evolutionary Stages. ZHANG X.-D., QIAN S.-B., ZHAO E.-G., et al.
2022MNRAS.514.5528L 19       D               6 33 ~ CoBiToM Project - II. Evolution of contact binary systems close to the orbital period cut-off. LOUKAIDOU G.A., GAZEAS K.D., PALAFOUTA S., et al.

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